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SessionName_LastName_PresentationTitle_Version# Massive star formation begins in cold and dense molecular clouds that undergo significant physical and chemical change during protostellar evolution. As the mass of the protostar grows, the stellar radiation heats and ionizes material in its immediate surroundings. Massive stars are also born predominately in dense clustered environments together with stars of lower stellar masses. These unique characteristics, coupled with strong feedback that massive young stars impart on their environment present a rich laboratory for astrophysics, as well as present challenges in unlocking these complex phenomena. In this presentation, I will review the progress that ALMA has brought to this field during its past 5 years of discovery. I'll highlight some questions that ALMA will (hopefully) tackle in the next 5 years.
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